Tel: 203-853-9444
Quotes: sales@bucksci.com
Cart 0
Scan-n-Search Infrared Software

Scan-n-Search Infrared Software


$1,850.00

Buck M500/M530 Compatible | Ease of Use | Free Support

Email sales@bucksci.com for detail

download "Scan-n-Search" IR Software for 30 Day Free Trial

 

Scan-n-Search Overview:

  • A complete program for handling Infrared data
  • A free viewer for infrared data
  • A free search program for FDM IR Reference Spectra Databases
  • Very easy to use, makes complex data manipulations simple
  • Powerful Batch-Processing automates repetitive tasks
  • Scaleable from the teaching lab to the on-line process environment
  • Extensible using the powerful open-source Python programming language
  • Reads and writes data in industry-standard file formats
  • Collects data directly from the M530 IR spectrophotometer

                   

                  Software Capabilities:

                  Step 1: In the M500/M530 start up screen, it checks your computer and network for all available drives so you can open and share to them.

                   

                  Step 2: In the Scan-n-Search is the polished instrument user interface that makes data collection a breeze. The single beam background scan is displayed and stored as the background for the sample runs to come.

                   

                  Step 3: In the Instrument Control Section, once the background Scan has been done, change to Sample mode and collect a real time %T scan of your sample. If you like the finished scan you can choose to save it, print it or do other advance manipulations on it.

                   

                  Step 4: Manual Peak Labeling at a click.

                   

                  Step 5: Advanced Functions Savitsky-Golay Smoothing for reduce system noise.

                   

                  Step 6: Advanced Functions - Library Search - Your Spectrum can be searched / compared against premade and libraries you construct.

                   

                  IR Reference Spectra Databases

                  An infrared spectrum of a molecule is like a fingerprint. By comparing the spectrum of an unknown compound to a library of data, the spectroscopist can identify the unknown. This technique has wide applications in many fields such as forensics, environmental chemistry, research, industrial quality control, and teaching.

                  Scan-n-Search Infrared Software includes a complete spectral library search tool with user-defined region searching, many search algorithms, and customizable reports.

                  Commercially available Reference Spectra Databases (Libraries)

                  Hundreds of Thousands of reference spectra are available from:

                      When ordering STJapan or NICODOM databases, specify the format to be "Galactic - Grams/32 & SpectralID".

                      Scan-n-Search Infrared Software can search any database from any source that is in "Galactic - Grams/32 & SpectralID" format.

                      Scan-n-Search Infrared Software can search WinFIRST libraries and Sadtler User Libraries, and can search against folders of individual files.

                       

                      Spectral Manipulations

                      • Zap Spectral Regions
                      • Zap spectral regions, with zeros or interpolated lines, with the capability of adding noise back into the zapped regions
                      • Manual Baseline Correction
                      • Automatic Baseline Correction
                      • Manual Spectral Subtraction
                      • X-Axis Shift and Stretch
                      • Take derivatives of spectral data
                      • FFT, ratio, absorbance, transmittance conversions
                      • FFT: Fast Fourier Transform of interferograms, with control over zero-filling, apodization and phase correction
                      • Convert data between Absorbance, Transmittance, and Diffuse Reflectance formats
                      • 5 to 99 point smoothing, with Savitsky-Golay, moving average, Hannig and Hamming window methods
                      • Interpolate / Decimate to change the resolution of the spectral data
                      • Manual Interactive Spectral Subtraction
                      • Automatic Spectral Subtraction optimized over a user-selected region
                      • Offset data by constant
                      • Scale data by constant
                      • Truncate to change the spectral data limits
                      • Kramers-Kroning transform using the Maclaurin method
                      • Raman Shift correction: with user supplied excitation frequency
                      • ATR Correction: Attenuated Total Reflectance correction with user control over angle of incidence and refractive indices
                      • Normalizations: Normalize the data to a minimum, a range, or using Vector Normalization
                      • Match spectra: set a group of spectra to have the same starting and ending values and number of data points

                                                                 

                                                                Synthesize Data

                                                                • Average / Add / Add with weights lists of individual datafiles to create new data
                                                                • Interactively add peaks to data by stretching data points
                                                                • Edit data: edit datapoints directly in a spreadsheet and instantly preview the result
                                                                • Create synthetic spectra from user-supplied peak tables with optional noise, baseline offset and baseline slope
                                                                • Generate Blackbody spectra with Radiance or Photon distribution for a given temperature
                                                                • Change header fields for corrupted or incorrectly converted files

                                                                           

                                                                          Data Analysis

                                                                          • Compute integrated areas of spectral regions
                                                                          • Peak Picking automatically tabulates the peaks in a spectrum
                                                                          • Manual Peak Picking and Labeling by right-clicking on a peak
                                                                          • Peak Measurement: computes peak height using user-supplied peak endpoints
                                                                          • Signal-to-Noise: computes signal-to-noise ratio over user-defined limits
                                                                          • User Library Search: search unknown spectra against libraries of data.

                                                                                    Share this Product


                                                                                    More from this collection

                                                                                    Questions & Answers

                                                                                    Have a Question?

                                                                                    Be the first to ask a question about this.

                                                                                    Ask a Question